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Statistics of Solar Filament Mass Based on CHASE Sun-as-a-star Spectroscopic Observations

  • Authors: T. Y. Xie, Z. H. Zhao, X. Cheng, Y. H. Chen, Z. Zheng, Q. Hao, C. Li, M. D. Ding

T. Y. Xie et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 3.

Geometric statistics and depth correction. (A) Distribution of the filament aspect ratio (L/Wapp). (B) Apparent width Wapp as a function of normalized heliocentric position x/R. The red curve shows the best-fit projection model (Equation (12)), yielding a depth-to-width ratio of a = 1.7. (C) Comparison between the apparent depth (assumed equal to Wapp) and the geometrically corrected depth DLOS, color encoded by heliocentric distance ∣x/R∣. The dashed line indicates the one-to-one correspondence.

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